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- W2108045889 abstract "Abstract We have carried out a large observational study of the radio luminosities, stellar populations, and environments of massive galaxies over the redshift range 0 < z < 1. Radio jets powered by an accreting central black hole are common in massive galaxies, and there is a large class of “optically quiet AGN,” with radio emission but no optical/IR signature of black-hole accretion. The central black holes in these galaxies are probably accreting in a radiatively inefficient mode, and our results suggest that “radio-mode feedback” as described by Croton et al . is likely to occur in all masssive early-type galaxies at z < 0.8. While it appears that radio-loud AGN occur episodically in all massive early-type galaxies, we also identify a sub-population of galaxies with powerful radio sources and a prominent younger (~ 10 8 yr) stellar population that may have undergone recent mergers." @default.
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- W2108045889 date "2009-08-01" @default.
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- W2108045889 title "Radio-Mode Feedback in Massive Galaxies at Redshift 0 < <i>z</i> < 1" @default.
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- W2108045889 doi "https://doi.org/10.1017/s1743921310006745" @default.
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